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E4411B
E4403B
E4408B
E4402B
E4404B
E4405B
E4407B
ESA Series
Spectrum
Analyzers
English URL
www.agilent.com/find/products
Economy Portable Spectrum Analyzer, ESA Series (cont.)
Signal Analysis
Wide Selection of Detectors
The ESA has a wide selection of detectors to meet all of your test
needs; including averaging (RMS), peak, negative peak, sample, and
quasi-peak (optional). Notably, the ESA’s RMS averaging detector
improves your measurement repeatability and efficiency when test-
ing noise like signals such as today’s 2G and 3G formats. In addition
the RMS detector provides RMS results as required by several stan-
dards. The ESA’s optional quasi-peak detector enables you to verify
your EMI performance of your DUT, making the ESA a flexible tool
for all types of design and verification testing. For a dedicated
EMI instrument with established measurement routines and EMI
software, the E7400A Series EMC precompliance analyzer may be
more appropriate.
Narrow Resolution Bandwidth Filters
Achieve the maximum frequency resolution with the ESA spectrum
analyzer’s optional narrow resolution bandwidths. The flexibility of
the ESA allows you to select the resolution that you need. The base
performance of the ESA includes a 1 kHz RBW. Add the narrow
resolution bandwidth option (1DR) to get 10 Hz minimum RBW’s
(100 Hz on the basic analyzer). Or, for the maximum performance,
order the high stability timebase option (1D5) in addition to the
narrow resolution bandwidth option to get 1 Hz RBW’s.
Measurements Made Easy
PowerSuite – Absolute Confidence in Making Power Measurements in
3 Easy Steps
The ESA simplifies the task of making common power measure-
ments through its built-in power measurements. These measure-
ment functions are easy to use.
Step 1
Press the measurement button on the front panel.
Step 2
Select the desired standards-based format or customize your test
setup.
The ESA includes a wide selection of standards-based test setups
including the following formats:
• cdmaOne (IS-95A/C)
• cdmaOne (J-STD-008)
• NADC
• GSM/GPRS and EDGE
• 3GPP W-CDMA TS 21.141 spurious emissions test
• W-CDMA 3GPP
• cdma2000 SR1
• cdma2000 SR3-MC
• cdma2000 SR3-DS
• PDC
•
Bluetooth
• TETRA
• WLAN 802.11a, b, g
• HiperLAN/2
• DVB-T
Step 3
Select the desired measurement functions.
The ESA offers the widest selection of built-in power measurements
available in a mid-range instrument:
• Channel power
• Occupied bandwidth
• Adjacent channel power (ACP)
• Multi-carrier ACP
• Power statistics (CCDF) (not available on the basic analyzer)
• Harmonic distortion
• Burst power
• Intermodulation distortion (TOI)
• Spurious emissions
• Spectrum
Agilent’s IO Libraries Suite
Agilent’s IO Libraries Suite ships with the ESA series spectrum
analyzers to help you quickly establish an error-free connection
between your PC and instruments – regardless of the vendor. It
provides robust instrument control and works with the software
development environment you choose. For additional description of
Agilent’s IO Libraries Suite features and installation requirements,
please go to
www.agilent.com/find/iosuite/data-sheet
IntuiLink PC Software
With IntuiLink software you can conveniently save and document
your results by linking the ESA to MS Word or Excel applications. In
addition, the IntuiLink software provides a simple programming
interface to the ESA spectrum analyzer allowing you to easily write
macros or functions within windows applications to control the ESA
spectrum analyzer. IntuiLink is included free of charge with
every ESA.
Remotely Control and Monitor the ESA over the Internet
BenchLink web remote control (Option 230) enables you to remote-
ly control your instrument over the internet or intranet. The
software operates on a locally-networked computer connected to
the ESA by GPIB. The ESA can then be controlled remotely from any
client computer on the internet or intranet with a standard
web browser.
Segmented Sweep
Segmented sweep allows you to view up to 32 discontinuous seg-
ments of the spectrum with varying levels of resolution at the same
time. This feature allows you to view problem spots at the same time
and save time while doing so by eliminating the need to retune or
make long sweeps (standard and communication test analyzers
only).
Log Sweep
The log sweep function on the ESA makes it very easy to set up limit
lines and view the spectrum in log scale. This is useful for meeting
test requirements, such as CISPR, that specify requirements on a log
scale (standard and communication test analyzers only).
Amplitude Corrections
Making amplitude corrections for cables, antennas, external mixers
or other peripherals used with the ESA is simple using the ESA’s
built-in amplitude correction tables. Simply populate the ESA’s
amplitude correction table with correction factors and then turn the
corrections on. Up to 4 correction tables may be loaded and applied
at any one time. Add correction factors for cables, antennas, or other
devices.
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